Ultraviolet-to-far infrared properties of Lyman break galaxies and luminous infrared galaxies at z ∼ 1

Astronomy and Astrophysics

Volumn 450, Issue 1, 2006, Pages 69-76

  Burgarella, D ^a   Perez Gonzalez P G ^b   Tyler, K D ^b   Rieke, G H ^b   Buat, V ^a   Takeuchi, T T ^a,i   Lauger, S ^a   Arnouts, S ^a   Ilbert, O ^c   Barlow, T A ^d   Bianchi, L ^e   Lee, Y W ^f   Madore, B F ^d,g   Malina, R F ^a   Szalay, A S ^h   Yi, S K ^f  

^a AIX MARSEILLE UNIVERSITÉ   (France)

^b UNIVERSITY OF ARIZONA   (United States)

^c INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e JOHNS HOPKINS UNIVERSITY   (United States)

^f Yonsei University   (South Korea)

^g CARNEGIE OBSERVATORIES   (United States)

^h JOHNS HOPKINS UNIVERSITY   (United States)

ⁱ TOHOKU UNIVERSITY   (Japan)

Author keywords

Cosmology: observations; Galaxies: evolution; Galaxies: fundamental parameters; Galaxies: starburst; Infrared: galaxies; Ultraviolet: galaxies

Indexed keywords

DUST; ESTIMATION; INFRARED RADIATION; LUMINESCENCE; SPACE RESEARCH; STATISTICAL METHODS; ULTRAVIOLET RADIATION;

COSMOLOGY: OBSERVATIONS; GALAXIES: EVOLUTION; GALAXIES: FUNDAMENTAL PARAMETERS; GALAXIES: STARBURST; INFRARED: GALAXIES; ULTRAVIOLET: GALAXIES;

GALAXIES;

EID: 33645822757     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054309     Document Type: Article

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